Fig. 8.
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Left: Gaia proper motions (PMs) of 83 group members of SPICY G342.1+0.2. The dashed ring marks the 1σ distribution of PMs from the centre of the group. The PMs of VVV-WIT-13 are obtained from the VIRAC2 catalogue of the VVV survey. The colour bar represents the difference between the PMs measured from Gaia and VVV. Right: PM distance of VVV-WIT-13 (black) and the 83 sources presented in the left panel.
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